The Solar Rotation in the 1930s from the Sunspot and Flocculi Catalogs of the Ebro Observatory

The tables of sunspot and flocculi heliographic positions included in the catalogs published by the Ebro Observatory in the 1930s have recently been recovered and converted into digital format by using optical character recognition (OCR) technology. We here analyzed these data by computing the angul...

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Detalles Bibliográficos
Autores: de Paula Vila, Víctor, Curto, Juan José, Casas, Ricard
Tipo de recurso: artículo
Fecha de publicación:2016
País:España
Institución:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repositorio:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:20.500.14342/5411
Acceso en línea:http://hdl.handle.net/20.500.14342/5411
https://doi.org/10.1007/s11207-016-0974-2
Access Level:acceso abierto
Palabra clave:Rotation
Active regions, velocity field
Sunspots, velocity
Solar cycle, observations
Descripción
Sumario:The tables of sunspot and flocculi heliographic positions included in the catalogs published by the Ebro Observatory in the 1930s have recently been recovered and converted into digital format by using optical character recognition (OCR) technology. We here analyzed these data by computing the angular velocity of several sunspot and flocculi groups. A difference was found in the rotational velocity for sunspots and flocculi groups at high latitudes, and we also detected an asymmetry between the northern and southern hemispheres, which is especially marked for the flocculi groups. The results were then fitted with a differential-rotation law [ω= a+ bsin 2B] to compare the data obtained with the results published by other authors. A dependence on the latitude that is consistent with former studies was found. Finally, we studied the possible relationship between the sunspot/flocculi group areas and their corresponding angular velocity. There are strong indications that the rotational velocity of a sunspot/flocculi group is reduced (in relation to the differential rotation law) when its maximum area is larger.